In the above equation the left-hand side depends on r and θ , while the right-hand side depends on z . The only way these two members are going to be equal for all values of r,θ and z is when both of them are equal to a constant. Let us define such a constant as −l2 .
With this choice for the constant, we obtain:
dz2d2Z−l2Z=0
The general solution of this equation is:
Z(z)=a1elz+a2e−lz
Such a solution, when considering the specific boundary conditions, will allow Z(z) to go to zero for z going to ±∞ , which makes physical sense. If we had given the constant a value of l2 , we would have had periodic trigonometric functions, which do not tend to zero for z going to infinity.
Once sorted the z -dependency, we need to take care of r and θ .
Again we are in a situation where the only way a solution can be found for the above equation is when both members are equal to a constant. This time we select a positive constant, which we call m2 . The equation for Θ becomes, then:
dθ2d2θ+m2θ=0
Its general solution can be written as:
θ(θ)=b1sin(mθ)+b2cos(mθ)
This solution is well suited to describe the variation for an angular coordinate like θ . Had we chosen to set both members of equation equal to a negative number, we would have ended up with exponential functions with a different value assigned to θ(θ) for each 360 degrees turn, a clear non-physical solution.
The equation (∗) is a well-known equation of mathematical physics called parametric Bessel's equation. With a simple linear transformation of variable, x=(k2+l2)r , equation (∗) is readily changed into a Bessel's equation:
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